to model the observations. Found since to work across all galaxies Ciardullo (03) ... for PNLF bright end in elliptical ( 10Gyr) galaxies? Possible explanations...
Term 'planetary nebula' coined by Herschel to describe faint, disk appearance ... falls directly to ground state, Lyman photon of sufficient energy to ionize ...
Asymmetric Planetary Nebulae IV. La Palma, Canary Islands. Water Fountains in Pre-Planetary Nebulae ... Outflow velocity of water masers extremely high ...
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Helium-3 in Planetary Nebulae. Bob Rood (UVa), Tom Bania (BU), Dana Balser (NRAO) ... PNe He3 at the VLA: Balser, Goss, Bania, Rood (2005) J320 3He Data. Model 35' ...
Good probes of stellar populations ... Absolute probes of stellar ... Intra-cluster (IC) PNs as probes of the IC starlight. PN morphology and stellar pops ...
Planetary Nebulae and the Extragalactic Distance Scale. Robin Ciardullo. Why Measure ... Collisional de-excitation of forbidden emission in young, dense nebulae ...
hydrodynamical calculations: large sets now becoming available. Perinotto ... Still to be included: full hydrodynamics, non-sphericity, binary progenitors, etc. ...
La Palma, Canary Islands. Kerttu Viironen, Antonio Mampaso ... Tenerife, Canary Islands. 2. Overview. The targets. Search method. Status of the analysis. ...
Preliminary modelling with CLOUDY. What is still to do ? Abundance analysis, Velocity field analysis, Archival IR data can be included for StWr 2-21. Project status : ...
Star Cluster a number of stars of common origin held together as a group by ... to a great short video about this irregular galaxy, called the 'Cigar Galaxy. ...
or at least the ejection process is strongly influenced by ... Hydra spectrograph, 2002-04. Dispersion 0.33 A/pix; resolution ~7500. RV precision ~3-3.7 km/s ...
Resonant cyclotron absorption in ion doped plasma (Hoshino et al 92, Amato ... RCA of ion cyclotron waves works effectively as an acceleration mechanism for ...
Serendipitous XMM-Newton Survey of Planetary Nebulae. Rodolfo Montez ... Hence, our search for serendipitously observed PNe in the vast XMM-Newton data archive. ...
Astronomical applications of spectroscopy: Planetary Nebulae. M57 ... Spectrum of M57 (different format) The energy level diagram of carbon (Grotian Diagram) ...
The newer telescopes (i.e.Gemini North/South) are being built to allow high ... Gemini North. Field of view: 11'' square. Colour-coded. intensity map. HST ...
Signatures of Magnetic Field Structure in Planetary Nebulae. P. J. ... 171 Angstrom. TRACE. strong field cases: longitudinal coherence. Molecular Clouds. gravity ...
Radio-to-X-ray diagnostics composition, energy transport, magnetic field geometry ... Example: The Mouse (Gaensler et al. 03) Radio X-ray synchrotron tails ...
Planetary Nebulae as a Testground of Interstellar Molecular Chemistry. Tatsuhiko Hasegawa ... Hasegawa & Kwok. Molecular Abundances and Densities from (sub-)mm ...
BUT the viewing and magnetic inclination angles can't be free parameters ... Brave Enough to Infer Magnetic Inclination Angle from Double Torus Separation, ...
A round or axisymmetric shape, sometimes with multiple shells or outer haloes. ... Silkworm. NGC 6302. Hb 5. Size does matter! 28. 28. A necessary question...
He created catalogs of double stars and nebulae; In 1800 he ... aliphatic (chain-like) C-H 'stretch' @ 3.4 mm. Gdansk 2005. 18. graphitic structure. NCAC ...
The CDS has put in place a system for advising on the structure for such ... For extragalactic PN actually residing in galaxies all the objects occur within ...
Totally weird. 39. Irregular. 3. Slow variations. 3. Eclipse. 3. Slow decline ... W-7405-Eng-48, the National Science Foundation through the Center for Particle ...
The ISO spectra of planetary nebulae (PNs) are characterized by ... Peculiar ... features, the dust continuum is of unknown origin and has a peculiar shape. ...
Pilyugin et. al (2003, A&A, 401, 557) find O/H = 8.52 dex in the solar vicinity ... was formed, there has been an 0.13 dex increase in oxygen abundance of the ISM ...
Reconstruction and Visualization of Planetary Nebulae Authors: M. Magnor, G. Kindlmann, C. Hansen, N. Duric Visualization II Instructor: Jessica Crouch
Rhys Morris, Bristol Astrophysics Group. For more information see http://www.star.bris.ac.uk ... Astrophysics Group. 2. Rhys Morris, Bristol Astrophysics Group ...
X-Ray Emission from Planetary Nebulae and Their Central Stars: A Status Report Joel Kastner Rochester Institute of Technology w/ help from lots of other folks, including:
... L pez et al. 1995) and fast, low ionization emission regions ... Assuming D= 860 /- 340 pc, the velocities of the ansae in the plane of the sky are: ...
40 ACS images of prePNe from Hubble archives thru 1996, WFPC2 being added. Color overlays of broadband images. Logarithmic intensities to enhance extended faint ...
... FOCAS data (218 PNs) in two fields partly overlapping the FORS data but ... Plus signs: absorption-line data. Squares: PN data. The. outer 4 points are based on ...
A. Rettura (ESO, IAP-Paris) S. S nchez (Calar Alto O bserv.) S. di Serego Allighieri (Arcetri, Italy) ... (ionization by the quasar) All along the radio axis ! ...
Physical conditions in shocked regions of ... Credit: NASA, ESA,HEIC, and the Hubble Heritage Team (STScI/AURA) ... A. Riera (UPC), P. Garc a-Lario (ESA) & ESA ...
... planetary nebulae as diagnostic probes for galaxy evolution ... How far are XPN useful probes for the study of resolved stellar populations in galaxies? ...
l (PAGB) / L(tot) = ? x Fuel. N(PN) / L(tot) = B x t. Fuel / L(hot-PAGB) N(PN) / M(tot) = B x t / (M/L) Renzini & Buzzoni (1986) Hot-PAGB Fuel Consumption ...